| . | Description . |
|---|---|
| par1 | Mass, black hole mass in solar masses |
| par2 | Dist, comoving (proper) distance in kpc |
| par3 | |$\log \dot{m}$|, |$\dot{m}=\dot{M}/\dot{M}_{\rm Edd}$| where |$\dot{M}_{\rm Edd}c^2=L_{\rm Edd}$| |
| par4 | rin, inner most radius of the accretion flow in rg |
| par5 | cos i, inclination angle of the disc |
| par6 | kTe, th, electron temperature for thermal corona in keV. If this parameter is negative, the model gives the inner hot Comptonization component. |
| par7 | kTe, nth, apparent electron temperature for non-thermal corona in keV which is recommended to be fixed at 300 keV to mimic non-thermal electron distribution. If this parameter is negative, the model gives the Comptonization component in the passive-disc corona region. |
| par8 | Γth, photon index of inner hot corona. If this parameter is negative then only the inner Compton component is used. |
| par9 | Γnth, photon index of disc-corona. If this parameter is negative, the model gives the outer disc. |
| par10 | fth, fraction of the hot Comptonizing component to the total Comptonization |
| par11 | rcor, outer radius of the disc-corona region in rg |
| par12 | log rout, outer radius of accretion disc in rg. If this parameter is −1, the code will use the self gravity radius as calculated from Laor & Netzer (1989) |
| par13 | redshift, must be fixed |
| par14 | fcol, switching parameter for colour correction (0: no colour correction, 1: colour correction factor is calculated by the same way as optxagnf (Done et al. 2012) |
| par15 | norm, must be fixed at 1 |
| . | Description . |
|---|---|
| par1 | Mass, black hole mass in solar masses |
| par2 | Dist, comoving (proper) distance in kpc |
| par3 | |$\log \dot{m}$|, |$\dot{m}=\dot{M}/\dot{M}_{\rm Edd}$| where |$\dot{M}_{\rm Edd}c^2=L_{\rm Edd}$| |
| par4 | rin, inner most radius of the accretion flow in rg |
| par5 | cos i, inclination angle of the disc |
| par6 | kTe, th, electron temperature for thermal corona in keV. If this parameter is negative, the model gives the inner hot Comptonization component. |
| par7 | kTe, nth, apparent electron temperature for non-thermal corona in keV which is recommended to be fixed at 300 keV to mimic non-thermal electron distribution. If this parameter is negative, the model gives the Comptonization component in the passive-disc corona region. |
| par8 | Γth, photon index of inner hot corona. If this parameter is negative then only the inner Compton component is used. |
| par9 | Γnth, photon index of disc-corona. If this parameter is negative, the model gives the outer disc. |
| par10 | fth, fraction of the hot Comptonizing component to the total Comptonization |
| par11 | rcor, outer radius of the disc-corona region in rg |
| par12 | log rout, outer radius of accretion disc in rg. If this parameter is −1, the code will use the self gravity radius as calculated from Laor & Netzer (1989) |
| par13 | redshift, must be fixed |
| par14 | fcol, switching parameter for colour correction (0: no colour correction, 1: colour correction factor is calculated by the same way as optxagnf (Done et al. 2012) |
| par15 | norm, must be fixed at 1 |
| . | Description . |
|---|---|
| par1 | Mass, black hole mass in solar masses |
| par2 | Dist, comoving (proper) distance in kpc |
| par3 | |$\log \dot{m}$|, |$\dot{m}=\dot{M}/\dot{M}_{\rm Edd}$| where |$\dot{M}_{\rm Edd}c^2=L_{\rm Edd}$| |
| par4 | rin, inner most radius of the accretion flow in rg |
| par5 | cos i, inclination angle of the disc |
| par6 | kTe, th, electron temperature for thermal corona in keV. If this parameter is negative, the model gives the inner hot Comptonization component. |
| par7 | kTe, nth, apparent electron temperature for non-thermal corona in keV which is recommended to be fixed at 300 keV to mimic non-thermal electron distribution. If this parameter is negative, the model gives the Comptonization component in the passive-disc corona region. |
| par8 | Γth, photon index of inner hot corona. If this parameter is negative then only the inner Compton component is used. |
| par9 | Γnth, photon index of disc-corona. If this parameter is negative, the model gives the outer disc. |
| par10 | fth, fraction of the hot Comptonizing component to the total Comptonization |
| par11 | rcor, outer radius of the disc-corona region in rg |
| par12 | log rout, outer radius of accretion disc in rg. If this parameter is −1, the code will use the self gravity radius as calculated from Laor & Netzer (1989) |
| par13 | redshift, must be fixed |
| par14 | fcol, switching parameter for colour correction (0: no colour correction, 1: colour correction factor is calculated by the same way as optxagnf (Done et al. 2012) |
| par15 | norm, must be fixed at 1 |
| . | Description . |
|---|---|
| par1 | Mass, black hole mass in solar masses |
| par2 | Dist, comoving (proper) distance in kpc |
| par3 | |$\log \dot{m}$|, |$\dot{m}=\dot{M}/\dot{M}_{\rm Edd}$| where |$\dot{M}_{\rm Edd}c^2=L_{\rm Edd}$| |
| par4 | rin, inner most radius of the accretion flow in rg |
| par5 | cos i, inclination angle of the disc |
| par6 | kTe, th, electron temperature for thermal corona in keV. If this parameter is negative, the model gives the inner hot Comptonization component. |
| par7 | kTe, nth, apparent electron temperature for non-thermal corona in keV which is recommended to be fixed at 300 keV to mimic non-thermal electron distribution. If this parameter is negative, the model gives the Comptonization component in the passive-disc corona region. |
| par8 | Γth, photon index of inner hot corona. If this parameter is negative then only the inner Compton component is used. |
| par9 | Γnth, photon index of disc-corona. If this parameter is negative, the model gives the outer disc. |
| par10 | fth, fraction of the hot Comptonizing component to the total Comptonization |
| par11 | rcor, outer radius of the disc-corona region in rg |
| par12 | log rout, outer radius of accretion disc in rg. If this parameter is −1, the code will use the self gravity radius as calculated from Laor & Netzer (1989) |
| par13 | redshift, must be fixed |
| par14 | fcol, switching parameter for colour correction (0: no colour correction, 1: colour correction factor is calculated by the same way as optxagnf (Done et al. 2012) |
| par15 | norm, must be fixed at 1 |
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